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Xref: cantaloupe.srv.cs.cmu.edu sci.astro:35223 sci.space:61404Newsgroups: sci.astro,sci.spacePath: cantaloupe.srv.cs.cmu.edu!das-news.harvard.edu!noc.near.net!howland.reston.ans.net!agate!ames!pan.arc.nasa.gov!mosesFrom: moses@pan.arc.nasa.gov (julie moses)Subject: Re: temperature of the dark skyMessage-ID: <1993Apr28.185206.3501@news.arc.nasa.gov>Sender: usenet@news.arc.nasa.govOrganization: NASA-Ames Research CenterReferences: <C65o4t.A7o@zoo.toronto.edu> <1993Apr28.002214.16544@Princeton.EDU>Date: Wed, 28 Apr 1993 18:52:06 GMTLines: 29>> Does anyone have a reference (something I can look up, not just your own>> recollections -- I have a few of those myself) on the temperature of the>> (night) sky as seen from space?>>>> Note, I am *not* talking about the temperature of the Microwave Background>> Radiation.  There are more things in the sky than just the MBR; what I'm>> after is total blackbody temperature -- what a thermal radiator would see,>> disregarding (or shielding against) the Sun and nearby large warm objects.>>I'm not sure if this will help you, but the (local) interstellarradiation field has been measured and modeled by various groups.  If Iremember things correctly, the models involved contributions from threedifferent BB sources, so there's no obvious "temperature" of backgroundradiation in our local area.  However, the following references give theinterstellar radiation density as a function of wavelength, and you canintegrate and average in an appropriate manner to get an "effective"temperature if you like:Witt and Johnson (1973) Astrophys. J. 181, 363 - 368Henry et al. (1980) Astrophys. J. 239, 859 - 866Mathis et al. (1983) Astron. Astrophys. 128, 212 - 229As you can see, the references are out of date, but they might get youstarted.Hope this helps,					Julie

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